Hybrid quenching model
*Coloured by host halo mass. All masses are in units of
Stellar-to-halo-mass relation
*All masses are in units of
Interactive Models
The purpose of this website is to understand the effect of the parameters of the stellar-to-halo-mass relation as well as those of the hybrid quenching model of galaxies from Behroozi et. al 2010 and Zu & Mandelbaum 2015, respectively.